The central region of the Milky Way is dominated by a bar - like structure, which stirs up the material in
the outer galactic disk as it rotates over millions of years and may be responsible for its spiral structure.
Not exact matches
However, their gravity has affected our Galaxy as well, distorting the
outer parts of the
galactic disk.
Moving out from this central
galactic bulge, the panorama sweeps from the galaxy's central bulge across lanes of stars and dust to the sparser
outer disk.
The rotation curve is flat in the
outer parts of most
galactic disks (dark matter!).
Some are found in globular clusters, but most move in a huge cloud around the
disk called the
galactic halo, which has a luminous inner component defined by globular star clusters and other easily observable stars (with coronae of hot gas possibly expelled by supernovae and of high - velocity neutron stars) and an
outer dark - matter component inferred from its gravitational impact on the Milky Way's spiral
disk.